A scan over 3σ neutrino parameters yields the most conservative lower bounds on the triplet-Higgs cubic coupling from μ→eγ, μ→3e, and μ-e conversion.
Measurement of the Total Active 8B Solar Neutrino Flux at the Sudbury Neutrino Observatory with Enhanced Neutral Current Sensitivity
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abstract
The Sudbury Neutrino Observatory (SNO) has precisely determined the total active (nu_x) 8B solar neutrino flux without assumptions about the energy dependence of the nu_e survival probability. The measurements were made with dissolved NaCl in the heavy water to enhance the sensitivity and signature for neutral-current interactions. The flux is found to be 5.21 +/- 0.27 (stat) +/- 0.38 (syst) x10^6 cm^{-2}s^{-1}, in agreement with previous measurements and standard solar models. A global analysis of these and other solar and reactor neutrino results yields Delta m^{2} = 7.1^{+1.2}_{-0.6}x10^{-5} ev^2 and theta = 32.5^{+2.4}_{-2.3} degrees. Maximal mixing is rejected at the equivalent of 5.4 standard deviations.
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Probing Type II Seesaw Leptogenesis Through Lepton Flavor Violation
A scan over 3σ neutrino parameters yields the most conservative lower bounds on the triplet-Higgs cubic coupling from μ→eγ, μ→3e, and μ-e conversion.